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ATEL # 2931; P.Balanutsa, E.Gorbovskoy, V.Lipunov, V.Kornilov, A.Belinski, N.Shatskiy, N.Tyurina, D.Kuvshinov, V.Chazov, A.Kuznetsov, D.Zimnukhov, M. Kornilov (SAI, Moscow), A. Tlatov, A.V. Parhomenko, D. Dormidontov (Kislovodsk solar station of the Pulkovo observatory RAS), V.Yurkov, Yu.Sergienko, D.Varda (Blagoveshchensk Educational University), V.Krushinski, I.Zalozhnih, T.Kopytova, A. Popov (Ural State University), K.Ivanov, S.Yazev, N.Budnev, E.Konstantinov, V.Lenok, O.Chuvalaev, V.Poleschuk, O.Gres,(Irkutsk State University)
on 13 Oct 2010; 10:47 UT
Distributed as an Instant Email Notice (Request for Observations)
Password Certification: Vladimir Lipunov (email@example.com)
Subjects: Optical, Request for Observations, Cataclysmic Variables, Transients, Stars
Referred to by ATEL #: 2938
MASTER auto-detection system at Kislovodsk detected a new transient source at the position (R.A., Dec) = 01h 53m 47.24s , +30d 38m 44s.0 (J2000) with a typical uncertainty of 0.2" at 2010-10-01 23:25:48 (UT).
The V magnitude is about 17.9 +-0.1 ( exposition 180s, m_lim = 19.0 ).
The OT is seen at next 7 images up 2010-10-12 in R and V. OT is blue: R-V=1.43 at 2010-10-01.9 .
There is no minor planet and any object brighter 21 mag in DSS at this place. We have a number images this field without OT. The last one was made at 2009-12-08 18:25:50 and have the limit V=19.4.
The nearest known galaxy is PGC1908869 (01h 53m 55.00s , +30d 33m 59.0s). The OT as the SN-candidate is relatively far and more brighter than possible host galaxy.
The spectral observations are needed.
The discovery image is available at http://observ.pereplet.ru/images/OT015347+303844/OT015347+303844.jpg
MASTER Robotic Net